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Asymptotic expansions of the null distributions of three test statistics in a nonnormal GMANOVA model

Hirokazu Yanagihara

(Received August 22, 2000) (Revised November 11, 2000)

Abstract. This paper deals with three test statistics for testing a linear hypothesis and estimators of regression coe½cients in the GMANOVA model which was proposed by Potthof and Roy (1964), without assuming normal error. The test statistics considered include the likelihood ratio statistic, the Lawley-Hotelling trace criterion and the Bartlett-Nanda-Pillai trace criterion, which have been proposed under normality. We obtain asymptotic expansions of the null distributions of three test statistics up to the ordernÿ1, wherenis the sample size. The results are generalizations of the formulas in Wakaki, Yanagihara and Fujikoshi (2000). In addition, asymptotic expansions of the distribution functions of several standardized statistics on regression coe½cients are derived.

1. Introduction

The GMANOVA model considered is de®ned by

Y ˆAXX0‡E; …1:1†

where Yˆ …y1;. . .;yn†0 is an np observation matrix of response variables, Aˆ …a1;. . .;an†0 is an nk between-individuals design matrix of explanatory variables with full rank k, X is a pq within-individuals design matrix of explanatory variables with full rank q …ap†, X is a kq unknown parameter matrix and Eˆ …e1;. . .;en†0 is an np error matrix. It is assumed that each vector ej is i.i.d., i.e., independently and identically distributed with E…ej† ˆ0 and Cov…ej† ˆS. This model can be applied to analysis of growth curve data, and hence it is also called the growth curve model.

We consider to test for a general linear hypothesis

H0:CXDˆO; …1:2†

where C is a known ck matrix with rank c …ak†, D is a known qd matrix with rank d …aq† andOis a cd matrix all of whose elements are 0.

2000 Mathematics Subject Classi®cation. primary 62H10, secondly 62E20.

Key words and phrases. Con®dence interval, Conservativeness, General multivariate linear hy- pothesis, Linear combination, MLE, Nonnormality, Robustness.

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The GMANOVA model (1.1) with normal error was introduced by Pottho¨ and Roy (1964) and have been extensively studied by many authors.

The maximum likelihood estimators X^ and S^ of X and S, and the likelihood ratio test statistic were obtained by Khatri (1966) and Gleser and Olkin (1970).

Fujikoshi (1974) studied properties of some test statistics, including the LR test statistic, and gave asymptotic expansions of their non-null distributions.

Gleser and Olkin (1970) were the ®rst to derive the exact density of MLE X. Asymptotic expansions of the distributions of^ X^ and its linear trans- form have been studied by Fujikoshi (1985, 1993a) and von Rosen (1997).

Various aspects of statistical inference under normality have been also discussed in literature. For these results, see. e.g., Kariya (1985), von Rosen (1991), Fujikoshi (1993b), Kshirsagar and Smith (1995), and Srivastava and von Rosen (1999).

The above results are based on the assumption that the error vectors e1;. . .;en are independently and identically distributed as a multivariate normal distribution with means 0 and covariance matrix S. Khatri (1988) discussed robustness for test statistic under elliptical distribution. However, the non- normal case has not been investigated so much, except for the case XˆIp, i.e., MANOVA case. For MANOVA case, Ito (1969, 1980), Chase and Bulgren (1971) and Everitt (1979) studied robustness of certain test statistics by simulation. Wakaki, Yanagihara and Fujikoshi (2000) obtained asymptotic expansions of the null distributions of three test statistics in nonnormal multivariate linear model. These results include several expansions obtained by Kano (1995), Fujikoshi (1997b, 2001), Fujikoshi, Ohmae and Yanagihara (1999) and Yanagihara (1999), as special cases. Our main purpose is to extend the asymptotic expansion formulas in a multivariate linear model to the ones in the GMANOVA model.

The present paper is organized in the following way. In O2, we describe three test statistics. It is shown that our test statistics can be expresses in terms of a random matrix U, which is a kind of Studentized version of X. Using^ this expression, we derive perturbation expansions of our test statistics. In O3, we give an asymptotic expansion of the distribution function of U. Further, asymptotic expansions of other standardized statistics of X^ are obtained in O4. In O5, we obtain asymptotic expansions of the null distributions of three test statistics, by expanding their characteristic function. Moreover, in O6, we discuss robustness of testing under nonnormality and derive a result on conservativeness based on the asymptotic expansion formulas. Some applica- tions of the asymptotic expansions of test statistics are given in O7. In O8, numerical accuracies are studied for some con®dence interval of X and asymptotic expansions of the null distributions for some test statistics under nonnormality.

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2. Test statistics and perturbation expansion

First, we summarize typical three test criteria that have been proposed under normality. LetShandSebe the variation matrices due to the hypothesis and the error, respectively, i.e.,

Shˆ …CXD†^ 0…CRC0†ÿ1…CXD†;^ SeˆD0…X0Sÿ1ÿ1D;

where

X^ˆ …A0ÿ1A0YSÿ1X…X0Sÿ1ÿ1;

Rˆ …A0ÿ1‡ …A0ÿ1A0YfSÿ1ÿSÿ1X…X0Sÿ1X†X0Sÿ1gY0A…A0ÿ1; and SˆY0…InÿPA†Y. Here PA is the projection matrix to the linear space R…A†generated by the column vectors of A. Then the following three criteria have been proposed, in particular, under normality.

(i) the likelihood ratio statistic:

TLRˆ ÿfnÿkÿ …pÿq† ‡s1glog…jSej=jSe‡Shj†;

(ii) the Lawley-Hotelling trace criterion:

THLˆ fnÿkÿ …pÿq† ‡s2gtr…ShSeÿ1†;

(iii) the Bartlett-Nanda-Pillai trace criterion:

TBNPˆ fnÿkÿ …pÿq† ‡s3gtrfSh…Sh‡Se†ÿ1g;

where the constantssj's are the Bartlett corrections in the normal case, and they are given as follows: s1ˆ ÿ…dÿc‡1†=2, s2ˆ ÿ…d‡1† and s3ˆc. For the special case qˆp, note that three criteria are reduced to the ones in the usual MANOVA model. Therefore, as in the MANOVA model, it may be sug- gested to use the criteria for nonnormal models.

Under normality, the distributions of these statistics have been extensively studied. Fujikoshi (1974) obtained asymptotic expansions of the non-null dis- tributions for three test statistics. Under nonnormality it is easily seen that the null distributions of these statistics converge towcd2 as the sample sizentends to in®nity under an appropriate regularity condition on the design matrix (see Huber (1973)). Our main purpose is to obtain asymptotic expansions of the null distributions of these statistics up to the order nÿ1 under a general condition.

Note that the three test statistics are invariant under the transformations from ‰Y0;XŠ to Sÿ1=2‰Y0;XŠ. Therefore, without loss of generality we may assume SˆIp by replacing X with Sÿ1=2X. In the following, we shall do that, and we regardX as Sÿ1=2X. We consider expressing the test statistics in terms of

Zˆ …A0ÿ1=2A0E; V ˆ 1

pnXn

jˆ1

…ejej0ÿIp†: …2:1†

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Note that …nÿ1ÿ1 can be expanded as 1

nS ÿ1

ˆIpÿ1 nV‡1

n…V2‡Z0Z† ‡Op…nÿ3=2†:

Therefore, 1

n…X0Sÿ1ÿ1

ˆ …X0ÿ1=2

Iq‡p …X1n 0ÿ1=2X0VX…X0ÿ1=2 ÿ1

n…X0ÿ1=2X0fV…IpÿPX†V‡Z0ZgX…X0ÿ1=2

…X0ÿ1=2‡Op…nÿ3=2†:

By using these results, we de®ne modi®ed matrices S~e, X~ and R~ by the fol- lowing relations, respectively.

1 nSe ÿ1

ˆ fD0…X0ÿ1Dgÿ1=2S~e2fD0…X0ÿ1Dgÿ1=2; X^ˆ …A0ÿ1=2ZXX…X~ 0ÿ1=2;

…A0ÿ1=2C0…CRC0†ÿ1C…A0ÿ1=2ˆRW~ R;~ where

Wˆ …A0ÿ1=2C0fC…A0ÿ1C0gÿ1C0…A0ÿ1=2:

Then, we obtain W2ˆW and get rank…W† ˆtr…W† ˆc. Further, the random matrices S~e, X~ and R~ can be expanded as

S~eˆIdÿ 1 2pnL0VL

‡ 1

2nL0 V IpÿPX‡3 4Q

V‡Z0Z

L‡Op…nÿ3=2†;

X~ˆIpÿ 1

p …In pÿPX†V

‡1

n…IpÿPX†fV…IpÿPX†V‡Z0Zg ‡Op…nÿ3=2†;

R~ˆIkÿ 1

2nWZ…IpÿPX†Z0W‡Op…nÿ3=2†;

…2:2†

where

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LˆX…X0ÿ1DfD0…X0ÿ1Dgÿ1=2;

QˆLL0ˆX…X0ÿ1DfD0…X0ÿ1Dgÿ1D0…X0ÿ1X0: Using these expressions, the three test statistics can be expanded as

TGˆtr…U0WU† ‡1

n‰fr1ÿkÿ …pÿq†gtr…U0WU†

‡r2trf…U0WU†2gŠ ‡Op…nÿ3=2†; …2:3†

where

UˆRZ~ XL~ S~e: …2:4†

Here the constants r1 and r2 are de®ned as follows;

…i† TLR :r1ˆs1; r2ˆ ÿ1=2;

…ii† THL :r1ˆs2; r2ˆ0;

…iii† TBNP:r1ˆs3; r2ˆ ÿ1:

In our derivation, ®rst we derive an asymptotic expansion of the distribution of U. Then, using the result, we obtain an asymptotic expansion of the null distribution of TG.

3. Edgeworth expansion of U

In this section, we obtain an asymptotic expansion of the distribution function of U up to the ordernÿ1. Without loss of generality, we assume that SˆIp as in a previous section. So, we regard X as Sÿ1=2X in the following expressions. Lete;e1;. . .;en be a sequence ofi.i.d.random vectors with E…e† ˆ 0 and Cov…e† ˆIp. We write a moment of e as

mi1...imˆE‰ei1. . .eimŠ;

where ej denotes the jth element of e. Similarly, the corresponding cumulant of e is expressed as ki1...im. Further, we use the following real matrix notation for arguments of some characteristic functions.

T ˆ ‰tabŠ:kd matrix;

T1ˆ ‰t…1†abŠ:kp matrix;

T2ˆ ‰…1‡dab†t…2†ab=2Š:pp matrix;

where dab is the Kronecker delta, i.e., daaˆ1 and dabˆ0 for a0b.

In order to get a valid expansion for the distribution function of U up the order nÿ1, we make some assumptions for the between-individuals design matrix A and the distribution of e. Let ln be the smallest eigenvalue ofA0A,

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and Mnˆmaxfkajk: jˆ1;. . .ng, where k k denotes the Euclidean norm.

We make the following assumptions.

B1. lim sup

n!y

1 n

Xn

jˆ1

kajk4<y, B2. lim inf

n!y

ln

n >0,

B3. For some constant d>0, MnˆO…n1=2ÿd†, B4. E…kek8†<y,

B5. The CrameÂr's condition for e and ee0; lim sup

ktk‡kT2k!yjE‰expfit0e‡itr…T2ee0†gŠj<1;

wheret is a p1 real vector. Here, we de®ne the norm of a matrix T2 as kT2k ˆ ‰Pp

aˆ1

Pp

bˆ1f…1‡dab†t…2†abg2=4Š1=2:

From (2.2) and (2.4), the random matrix U can be expanded as UˆU0‡ 1

pnU1‡1

nU2‡Op…nÿ3=2†; …3:1†

where

U0ˆZL;

U1ˆ ÿ1

2ZfQ‡2…IpÿPX†gVL;

U2ˆ1

8Z‰2fQ‡2…IpÿPX†gVfQ‡2…IpÿPX†g ‡QVQŠVL

‡1

2ZfQ‡2…IpÿPX†gZ0ZLÿ1

2WZ…IpÿPX†Z0WZL:

Using (3.1), the characteristic functionCU…T†ofU can be expanded under the assumptions B1, B2, B3 and B4 as

CU…T† ˆE‰expfitr…T0U†gŠ

ˆE‰expfitr…T0U0†gŠ ‡ 1

pnE‰itr…T0U1†expfitr…T0U0†gŠ

‡1

nE itr…T0U2† ‡i2

2ftr…T0U1†g2

expfitr…T0U0†g

‡o…nÿ1†

ˆCU…0†…T† ‡ 1

pnCU…1†…T† ‡1

nC…2†U …T† ‡o…nÿ1†:

Now we need to evaluate each term in the expansion ofCU…T†. Here we note that, rank…L† ˆd, which can be essentially done in the same way as in Wakaki, Yanagihara and Fujikoshi (2000). The method is based on the use of dif- ferentials for C…T1;T2†, which is de®ned by

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C…T1;T2† ˆE‰expfitr…T10Z‡nÿ1=2T2V†gŠ:

Therefore, letting T1ˆTL0 we have CU…0†…T† ˆC…T1;O†

ˆexp (i2

2 tr…T10T1† ‡ i3 6 

pn Xk

a0b0c0

Xp

abc

t…1†a0at…1†b0bt…1†c0cwa0b0c0kabc

‡ i4 24n

Xk

a0b0c0d0

Xp

abcd

t…1†a0at…1†b0bt…1†c0ct…1†d0dwa0b0c0d0kabcd ‡o…nÿ1† )

;

where

wa1...aj ˆ1 n

Xn

iˆ1

Yj

lˆ1

wial; 

pn

…A0ÿ1=2aiˆ …wi1;. . .;wik†0: …3:2†

Further,

CU…1†…T† ˆ ÿi

2E‰trfT0Z…Q‡2…IpÿPX†VLgexpfitr…T0ZL†Šg

ˆ ÿi

2E‰trfT10Z…Q‡2…IpÿPX††Vgexpfitr…T10Z†gŠ

ˆ ÿi

2…i†ÿ2Xk

a0

Xp

abc

t…1†a0c…qab‡2rab† q2

qt…1†a0aqt…2†bc C…T1;T2†jT2ˆO; …3:3†

where qab and rab the …a;b†th elements of Q and IpÿPX resrpectively, and Pk

a1...aj ˆPk

a1ˆ1. . .Pk

ajˆ1. Note that q2

qt…1†a0aqt…2†bc C…T1;T2†jT2ˆO

ˆ

"

i2wa0kabc‡i4t…1†a0a

Xk

b0

Xp

d

t…1†b0dwb0kbcd

‡ 1

pn (

i3Xp

d

t…1†a0d…mabcdÿdaddbc† ‡i5 2t…1†a0a

Xk

b0

Xp

de

t…1†b0dt…1†b0e…mbcdeÿdbcdde†

‡i5 2

Xk

b0c0d0

Xp

def

t…1†b0et…1†c0ft…1†d0dwa0b0c0wd0kaefkbcd )#

C…T1;O† ‡o…nÿ1=2†:

Moreover, it holds that …IpÿPX†Lˆ0, tr…IpÿPX† ˆ pÿq, …IpÿPX†2ˆ IpÿPX, L0LˆId and Q2ˆQ, in other words

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Xp

b

ˆrablbjˆ0; Xp

a

raaˆ pÿq; Xp

c

racrbcˆrab; Xp

a lailajˆdij; Xp

c qacqbcˆqab;

where lab is the …a;b†th element of L. By substituting these equations into (3.3) and replacing t…1†a0a with Pd

jˆ1ta0jlaj, we can evaluate CU…0†…T† and CU…1†…T†.

Similarly, we can evaluate CU…2†…T†. Therefore, we can obtain an expansion of CU…T†, whose formal inversion yields a valid expansion of the distribution function of U as in the following Theorem 3.1.

Some additional notations on cumulants need to be de®ned before describing Theorem 3.1. The quantity K…laq1q1†, which depends on the third order cumulants and the elements of L and Q is de®ned as

K…laq1q1†ˆ Xp

a0b0c0

la0aqb0c0ka0b0c0: …3:4†

In this expression, the order of indices inK corresponds to the one of indices in ka0b0c0. So, the l accompanying with index a0 appears to the ®rst order of indices in K. Similarly, the second and third order of indices in K are the q with indices b0 and c0, respectively. Further, the same number in indices expresses as the same element of symmetric matrix. Along the same line as (3.4), we de®ne

K…lar1r2†…lbr1r2†ˆ Xp

a0b0c0d0e0f0

la0ald0brb0e0rc0f0ka0b0c0kd0e0f0: Other constants are de®ned similarly.

Theorem 3.1. Suppose that the design matrix A and the error matrix Ein (1.1) satisfy the assumptions B1,B2,B3,B4 and B5. Let uˆvec…U†, then the distribution function of U can be expanded as

P…vec…U†ax†

ˆ …x1

ÿy. . . …xkd

ÿyfkd…u† 1‡ 1

pnR1…u† ‡1 nR2…u†

du‡o…nÿ1†;

where

R1…u† ˆ ÿ1 2

Xk

a0

Xd

ab

wa0…K…laq1q1†‡2K…lar1r1††Ha0a…u†

‡1 6

Xk

a0b0c0

Xd

abc

…wa0b0c0ÿ3wa0db0c0†K…lalblc†Ha0a;b0b;c0c;d0d…u†; …3:5†

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R2…u† ˆ1 8

Xk

a0b0

Xd

abcd

wa0wb0…K…laq1q1†…lbq2q2†‡3K…lalbq1†…q1q2q2†

‡4K…laq1q2†…lbq1q2†‡4K…lar1r1†…lbr2r2†‡8K…lalbr1†…r1r2r2†

‡12K…lar1r2†…lbr1r2†‡4K…lalbr1†…q1q1r1†‡12K…laq1r1†…lbq1r1†

‡4K…lalbq1†…q1r1r1†‡4K…laq1q1†…lbr1r1††Ha0a;b0b…u†

‡1 2

Xk

a0

Xd

a

f…k‡3pÿ2q‡1† ‡oa0a0…pÿq†gHa0a;a0a…u†

‡ 1 24

Xk

a0b0c0d0

Xd

abcd

‰…wa0b0c0d0ÿ3da0b0dc0d0†K…lalblcld†

ÿ2wa0b0c0wd0fK…lalblc†…ldq1q1†‡3K…laldq1†…lblcq1†

‡2K…lalblc†…ldr1r1†‡6K…laldr1†…lblcr1†g ‡3wa0wb0dc0d0fK…laq1q1†…lblcld†

‡K…lalbq1†…lcldq1†‡2K…lalcq1†…lbldq1†‡4K…lar1r1†…lblcld†

‡4K…lalbr1†…lcldr1†‡8K…lalcr1†…lbldr1†g

‡6da0b0dc0d0dacdbcŠHa0a;a0b;c0c;d0d…u†

‡ 1 72

Xk

a0b0c0d0e0f0

Xd

abcbdef

…wa0b0c0wd0e0f0ÿ6wa0b0c0wd0de0f0‡9wa0db0c0wd0de0f0†

K…lalblc†…ldlelf†Ha0a;b0b;c0c;d0d;e0e;f0f…u†: …3:6†

Here fkd…u† is the probability density function of Nkd…0;Ikd† given by fkd…u† ˆ …2p†ÿkd=2exp…ÿu0u=2†, and Ha10a1;...;aj0aj…u†is the multivariate Hermite polynomial.

In Theorem 3.1, the multivariate Hermite polynomial is de®ned by Ha10a1;...;aj0aj…u† ˆ …ÿ1†j qj

qua10a1. . .quaj0aj

fkd…u†;

where ua0a is the …a0;a†th element of U. For example Ha0a…u† ˆua0a;

Ha0a;b0b…u† ˆua0aub0bÿdabda0b0;

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Ha0a;b0b;c0c…u† ˆua0aub0buc0cÿX

‰3Š

ua0adbcdb0c0;

Ha0a;b0b;c0c;d0d…u† ˆua0aub0buc0cud0dÿX

‰6Š

ua0aub0bdcddc0d0‡X

‰3Š

dabdcdda0b0dc0d0; Ha0a;b0b;c0c;d0d;e0e;f0f…u† ˆua0aub0buc0cud0due0euf0f ÿX

‰15Š

ua0aub0buc0cud0ddefde0f0

‡X

‰45Š

ua0aub0bdcddefdc0d0de0f0‡X

‰45Š

dabdcddefda0b0dc0d0de0f0: Here P

‰ means the sum of all j possible combinations of the sets ai0 and ai, for example

X

‰3Š

da0b0dc0d0dabdcd ˆda0b0dc0d0dabdcd‡da0c0db0d0dacdbd‡da0d0db0c0daddbc: It may be noted that we can demonstrate the validity of the expansion by the argument similar to the one as in Wakaki, Yanagihara and Fujikoshi (2000), which is based on the same manner as in Bhattacharya and Ghosh (1978). Moreover, the moment condition B4 will be replaced with E…kek4†<

y as in Hall (1987).

4. Asymptotic expansions of the distribution functions of X^ and its linear combination

4.1. Two types of standardizations

In this section we consider asymptotic expansions of the distribution functions for X^ and its linear combination, where X^ is the maximum like- lihood estimator of X under normality. Related to the construction of con®- dence intervals ofXand its linear combination, we consider following two types of standardizations.

(1) standardized X:^

US ˆ …A01=2…X^ÿX†…X0Sÿ11=2; (2) Studentized X:^

UTˆ 

pn

…A01=2…X^ÿX†…X0Sÿ11=2; (3) standardized linear combination of X:^

USL ˆa0…X^ÿX†b=t;

(4) Studentized linear combination of X:^ UTLˆa0…X^ÿX†b=^t;

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where a and b are k1 and q1 ®xed vectors, respectively, and positive values t and ^t are de®ned by

t2ˆa0…A0ÿ1ab0…X0Sÿ1ÿ1b; ^t2ˆ1

na0…A0ÿ1ab0…X0Sÿ1ÿ1b:

Note that these standardizations have been proposed under normality.

However, we shall see that such standardizations do work asymptotically under nonnormality. Under normality, Fujikoshi (1987, 1993a) and von Rosen (1997) derived asymptotic expansions of the distributions of these statistics.

Further, its error bounds were discussed in Fujikoshi (1987, 1993a).

In this section, without loss of generality, we assume that SˆIp as in previous sections. So, X is regarded asSÿ1=2X. Therefore, t2 is rewritten as

t2 ˆa0…A0ÿ1ab0…X0ÿ1b:

4.2. Asymptotic expansion of US

Let MˆX…X0ÿ1=2 whose …a;b†th elements of M is denoted as mab. From (2.1), US can be expanded as

US ˆZMÿ 1

pnZ…IpÿPX†VM

‡1

nZ…IpÿPX†fV…IpÿPX† ‡Z0ZgM‡Op…nÿ3=2†: …4:1†

From (4.1) we can expand the characteristic function CUS…T3† of US as CUS…T3† ˆE‰expfitr…T30ZM†gŠ

ÿ i

pnE‰trfT30Z…IpÿPX†VMgexpfitr…T30ZM†gŠ

‡i

nE‰trfT30Z…IpÿPX†fV…IpÿPX† ‡Z0ZgMgexpfitr…T30ZM†gŠ

‡i2

2nE‰ftr…T30Z…IpÿPX†VM†g2expfitr…T30ZM†gŠ ‡o…nÿ1†;

where T3 is a kq real matrix. Letting T1ˆT3M0, we can see that the characteristic function can be evaluated by the same method as in Section 3.

In this case, using the relations M0MˆIq, MM0ˆPX and …IpÿPX†M ˆ0, we can obtain an expansion of CUS…T3†, whose inversion yields an asymptotic expansion of the distribution function of US as in Theorem 4.1.

Theorem 4.1. Suppose that the design matrix A and the error matrix Ein (1.1)satisfy the assumptions B1,B2,B3,B4and B5. Let uˆvec…US†, then the distribution function of US can be expanded as

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P…vec…US†ax†

ˆ …x1

ÿy. . . …xkq

ÿyfkq…u† 1‡ 1

pnRS;1…u† ‡1 nRS;2…u†

du‡o…nÿ1†;

where

RS;1…u† ˆ ÿXk

a0

Xq

a

wa0K…mar1r1†Ha0a…u†

‡1 6

Xk

a0b0c0

Xq

abc

wa0b0c0K…mambmc†Ha0a;b0b;c0c…u†; …4:2†

RS;2…u† ˆ1 2

Xk

a0b0

Xq

ab

‰…pÿq†da0b0dabÿda0b0K…mambr1r1†

‡wa0wb0fK…mar1r1†…mbr2r2†‡2K…mambr1†…r1r2r2†

‡3K…mar1r2†…mbr1r2†gŠHa0a;b0b…u†

‡ 1 24

Xk

a0b0c0d0

Xq

abcd

‰12wa0wb0dc0d0K…mamcr1†…mbmdr1†

ÿ4wa0b0c0wd0fK…mambmc†…mdr1r1†‡3K…mambr1†…mcmdr1†g

‡wa0b0c0d0K…mambmcmd†ŠHa0a;b0b;c0c;d0d…u†

‡ 1 72

Xk

a0b0c0d0e0f0

Xq

abcdef

wa0b0c0wd0e0f0

K…mambmc†…mdmemf†Ha0a;b0b;c0c;d0d;e0e;f0f…u†: …4:3†

Specially, when e is distributed as Np…0;S†, RS;1…u† ˆ0; RS;2…u† ˆ1

2…pÿq†Xk

a0

Xq

a

Ha0a;a0a…u†:

Therefore,

P…vec…US†ax†

ˆ …x1

ÿy. . . …xkq

ÿyfkq…u† 1‡ 1

2n…pÿq†Xk

a0

Xq

a

Ha0a;a0a…u†

" #

du‡o…nÿ1†:

This result coincides with the formula in Fujikoshi (1987).

(13)

4.3. Asymptotic expansion of UT

Let li be the eigenvalues of X0X and Lˆdiag…l1;. . .;lq†. Further, let H be an orthogonal matrix of orderq such that …X0X† ˆHLH0. Then, using a perturbation formula (see, Okamoto and Fujikoshi (1976)), we have

n

p …X0Sÿ11=2ˆ …X01=2‡p1nHS…1†H0‡1

nHS…2†H0‡Op…nÿ3=2†; …4:4†

where the …i;j†th elements of S…1† and S…2† are de®ned by …S…1††ijˆ …B†ij

li p ‡ 

lj

p ; …S…2††ijˆ ÿ …S…1†2†ij

li p ‡ 

lj p :

Here …†ij is denoted as the …i;j†th element of the matrix in the parenthesis and the matrix B is de®ned by

Bˆ ÿH0X0 Vÿp …V1n 2‡Z0

XH:

Substituting (4.4) into UT, we can represent as UT ˆUS‡ 1

pnUS…X0ÿ1=2HS…1†H0

‡1

nUS…X0ÿ1=2HS…2†H0‡Op…nÿ3=2†: …4:5†

From (4.5), the characteristic function CUT…T3† of UT can be expanded as CUT…T3† ˆCUS…T3†

‡ i

pnE‰trfT30…X0ÿ1=2HS…1†H0gexpfitr…T30US†gŠ

‡i

nE‰trfT30…X0ÿ1=2HS…2†H0gexpfitr…T30US†gŠ

‡i2

2nE‰ftrfT30…X0ÿ1=2HS…1†H0gg2expfitr…T30US†gŠ ‡o…nÿ1†:

By computing CUT…T3† and inverting the resultant expansion, we can obtain an asymptotic expansion of UT as in Theorem 4.2.

Theorem 4.2. Suppose that the design matrix A and the error matrix Ein (1.1) satisfy the assumptions B1, B2, B3, B4 and B5. Let uˆvec…UT†,

hijˆ  1 li p ‡ 

lj

p ; nijˆhij li;

and hab, h…1†ab and h…2†ab denote the …a;b†th elements of H, XH and …X01=2H respectively. Then the distribution function of UT can be expanded as

Table 6.1: Actual test sizes of the one-way ANOVA test for several a 1 and k 4
Table 6.2: Actual test sizes of the one-way ANOVA test for several a 1 , a 2 , k 3 and k 4
Table 8.1 gives the following six probabilities on one-side 90%, 95% and 99% con®dence intervals.
Table 8.1: Actual probabilities for con®dence intervals of a 0 Xb
+5

参照

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Key words and phrases: Linear positive operators, Summation-integral type operators, Rate of convergence, Asymptotic for- mula, Error estimate, Local direct results,